Table 14.

Values of Nside for foreground parameter variations in three different 20% large regions of the sky. The Nside values are chosen to capture most of the spatial variability of the spectral indices and to keep the resulting foreground bias under control while not increasing the statistical uncertainty. The angular resolution for βd is kept to the maximum allowed (Nside = 64), since LiteBIRD turns out to be particularly sensitive to this parameter.

Galactic latitude
LowMediumHigh
βd646464
Td840
βs422
Galactic latitude
LowMediumHigh
βd646464
Td840
βs422
Table 14.

Values of Nside for foreground parameter variations in three different 20% large regions of the sky. The Nside values are chosen to capture most of the spatial variability of the spectral indices and to keep the resulting foreground bias under control while not increasing the statistical uncertainty. The angular resolution for βd is kept to the maximum allowed (Nside = 64), since LiteBIRD turns out to be particularly sensitive to this parameter.

Galactic latitude
LowMediumHigh
βd646464
Td840
βs422
Galactic latitude
LowMediumHigh
βd646464
Td840
βs422
Close
This Feature Is Available To Subscribers Only

Sign In or Create an Account

Close

This PDF is available to Subscribers Only

View Article Abstract & Purchase Options

For full access to this pdf, sign in to an existing account, or purchase an annual subscription.

Close